! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template ! $Id: 6767,v 11.1 1997/04/09 19:54:15 pepsa Exp $ ! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template ! $Id: 6767,v 11.1 1997/04/09 19:54:15 pepsa Exp $ ! ! Refer to the HST Phase II Proposal Instructions to fill this out ! ! Anything after a "!" is ignored, and may be deleted ! ! All keywords with multiple entries are comma delimited except the ! Visit_Requirements and Special_Requirements keywords which can be ! delimited with carriage returns or semi-colons, but not commas ! ! For help call your Program Coordinator: Ready ! Phone: 410-338-4546 , E-mail: ready@stsci.edu ! ! This partially completed template was generated from a Phase I proposal. ! Name of Phase I Proposal: archive-0973.rosenthal.prop ! Date generated: Fri Dec 22 17:46:33 EST 1995 ! Proposal_Information ! Section 4 Title: A Search for Brown Dwarfs and Luminous Young Planets in the Hyades Proposal_Category: GO Scientific_Category: COOL STARS Cycle: 6 Investigators PI_name: Edward Rosenthal PI_Institution: Harvard-Smithsonian Center for Astrophysics CoI_Name: Todd Henry CoI_Institution: Space Telescope Science Institute Contact: N CoI_Name: Michael Skrutskie CoI_Institution: University of Massachusetts/Amherst Contact: N CoI_Name: Iain Neill Reid CoI_Institution: California Institute of Technology Contact: N Abstract: ! Free format text (please update) We propose to continue a photometric search for very low- temperature (~ 1200 K) brown dwarfs and luminous, young planets as companions to 20 low-mass stars in the Hyades. The Planetary Camera will be used to obtain 1-Mum images of the primary stars in order to search for faint companions. We were awarded 8 stars for Cycle 5 in HST proposal GO-6137. The initial reduced data are presented here and answer the previous concerns of the Cool Stars Panel with respect to feasibility. We would now like to observe the remaining 12 stars from our original target list in order to obtain a more robust statistical sample. We are undertaking a complementary project at the NASA IRTF involving imaging at J (1.2 Mum), H (1.6 Mum), and K (2.2 Mum) for a sample of 75 low-mass Hyades stars, including these 20 HST stars. The IRTF search will be more sensitive, but will also have much poorer spatial resolution. Since a large fraction of stellar companions are within 10 AU of their primary (Henry 1991), and at the distance of the Hyades 0."1 ~ 5 AU, the guaranteed 0."1 spatial resolution of the PC is crucial for this project. Similar I-band Cycle 4-6 programs are also underway (e.g. SNAP- 5353/Reid), although aimed at detecting low-mass stellar companions in a larger sample. Our program will go deeper by 2 magnitudes, by using the 1-Mum (vs I-band) filter and by taking longer effective exposures. This push to fainter luminosities is substantial considering the large uncertainties associated with current brown dwarf models. Questions ! Free format text (please update) Observing_Description: We propose a search for very low-mass companions (brown dwarfs/superplanets) to 12 low-mass M dwarfs in the Hyades cluster. We will image using the Planetary Camera (WFPC2/PC1) and the F1042M filter. Each target star will be imaged either 2 or 4 times in a single orbit; 12 target stars will thus require 12 orbits of HST observing time. This proposal is an extension of our Cycle 5 program GO-6137. For Cycle 5 we originally proposed for 20 target stars and were awarded 8 stars; all 8 of those stars have been observed in Cycle 5. The remaining 12 stars for which we are now proposing will complete our initial Hyades survey. The visibility period for the Hyades is 53 min; allowing 12 min for the guide star acquisition leaves 41 min on-source time per orbit. Based on experience with our Cycle 5 data thus far, we will likely take 2 1100-sec exposures per star, which should allow for adequate cosmic ray removal while not saturating on the primary star. If this procedure seems too risky (our Cycle 5 data are still being analyzed) then we will instead take 4 400-sec exposures per star, as we have already done with our first 6 Cycle 5 Hyades targets. These estimates assume that we continue to use SPATIAL SCANs (vs POS TARGs) for 4 exposures/orbit, which yield a reduced overhead of ~ 5 min total per read. Probably we will do 2 exposures/star. We will continue to sub-pixel dither if we choose 4 exposures/star, in order to improve photometric accuracy and spatial information, although for 2 exposures/star the added difficulty associated with cosmic ray removal indicates that integer-pixel dithering (in that case the primary aim is to avoid cosmetic defects on the chip) would be best. The final processed image frames will be corrected for cosmic rays, registered, and coadded. A model psf will be subtracted from the final images and the resulting final frame for each star will be compared with a Richardson-Lucy-Hook deconvolution in order to search for faint companions. Twenty target stars have been selected in total for this project because there are only ~ 20 RHY stars faint enough so as not to saturate the PC within our exposure times. While not a strict requirement, not saturating on the primary allows it to be used as a photometric check and also allows for companions to be detected as close to the primary as possible, considering the noise and Tiny Tim systematic modeling errors associated with the psf. Also, 20 total orbits keeps this observing program small while still providing a good statistical sample. If the Hyades brown dwarf distribution is similar to that of low-mass stellar companions to nearby field stars, then for 20 stars we would expect to detect ~ a few candidate substellar companions (Henry 1991). Each target star will require 1 orbit to complete its observations. These new observations will not only augment our existing Cycle 5 data but will also support the images of Reid's Cycle 4-6 SNAP programs. While the SNAP programs are geared to better determining what fraction of stars are binary with stellar companions, this proposal is aimed at imaging as deep and red as possible for a subset of the SNAP sample in order to search for brown dwarfs/superplanets. In addition, our F1042M filter overlaps with the shortest bandpass filter for NICMOS, allowing for a more direct comparison of our data with probable future NICMOS images. Real_Time_Justification: None. Supporting HST observations have been obtained for the first 8 stars in our Hyades sample during Cycle 5 (GO-6137). Supporting ground-based observations have been obtained with the NASA IRTF, Mauna Kea, during 1994 and 1995. Additional ground-based infrared observations of Hyades stars are being carried out at the Keck telescope by MacIntosh and Zuckerman (MacIntosh, personal communication, 1995). The IRTF/Keck observations are in the near-infrared, at J (1.2 micron), H (1.6 micron), and K (2.2 micron). Because these images will be closer to the peak of the spectral energy distribution of very cool companions, they will go deeper than the HST observations proposed here, but with a trade-off of poorer spatial resolution. Since the majority of companions are expected to fall within ~ 0."25 at the distance of the Hyades (Henry 1991), the diffraction-limited spatial resolution of HST provides a critical additional measure of the Hyades low- mass binary fraction. Calibration_Justification: ! Move appropriate text from Real_Time_Justification Additional_Comments: Fixed_Targets ! Section 5.1 Target_Number: 1 Target_Name: RHY067 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 07M 24.4S +/- 0.06S, DEC=10D 44' 15" +/- 1.0" PLATE-ID=01X0 ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1983.84 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 17.93, ! Include at least V and B-V I = 14.61 Comments: from RHY sample Target_Number: 2 Target_Name: RHY080 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 09M 27.7S +/- 0.06S, DEC=19D 18' 15" +/- 1.0" PLATE-ID=000O ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 17.94, ! Include at least V and B-V I = 14.77 Comments: from RHY sample Target_Number: 3 Target_Name: RHY083 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 09M 57.0S +/- 0.06S, DEC=16D 22' 42" +/- 1.0" PLATE-ID=000O ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 17.44, ! Include at least V and B-V I = 13.94 Comments: from RHY sample Target_Number: 4 Target_Name: RHY098 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 12M 03.2S +/- 0.06S, DEC=20D 49' 53" +/- 1.0" PLATE-ID=000O ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 16.61, ! Include at least V and B-V I = 13.41 Comments: from RHY sample Target_Number: 5 Target_Name: RHY110 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 13M 54.0S +/- 0.06S, DEC=15D 50' 09" +/- 1.0" PLATE-ID=000O ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 16.78, ! Include at least V and B-V I = 13.75 Comments: from RHY sample Target_Number: 6 Target_Name: RHY115 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 14M 45.0S +/- 0.06S, DEC=19D 03' 51" +/- 1.0" PLATE-ID=000O ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 16.55, ! Include at least V and B-V I = 13.47 Comments: from RHY sample Target_Number: 7 Target_Name: RHY126 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 16M 13.4S +/- 0.06S, DEC=16D 47' 48" +/- 1.0" PLATE-ID=000O ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 17.35, ! Include at least V and B-V I = 13.88 Comments: from RHY sample Target_Number: 8 Target_Name: RHY166 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 21M 48.9S +/- 0.06S, DEC=09D 50' 45" +/- 1.0" PLATE-ID=002J ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.80 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 17.11, ! Include at least V and B-V I = 14.32 Comments: from RHY sample Target_Number: 9 Target_Name: RHY199 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 24M 20.8S +/- 0.06S, DEC=19D 10' 52" +/- 1.0" PLATE-ID=000P ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 16.68, ! Include at least V and B-V I = 13.48 Comments: from RHY sample Target_Number: 10 Target_Name: RHY202 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 24M 30.5S +/- 0.06S, DEC=18D 59' 14" +/- 1.0" PLATE-ID=000P ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.96 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 16.68, ! Include at least V and B-V I = 13.35 Comments: from RHY sample Target_Number: 11 Target_Name: RHY254 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 27M 51.75S +/- 0.06S, DEC=09D 51' 18" +/- 1.0" PLATE-ID=002J ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.80 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 16.34, ! Include at least V and B-V I = 13.33 Comments: from RHY sample Target_Number: 12 Target_Name: RHY297 Alternate_Names: Description: STAR, M V-IV Position: RA=04H 31M 12.5S +/- 0.06S, DEC=12D 28' 38" +/- 1.0" PLATE-ID=002J ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox: J2000 RV_or_Z: RA_PM: 0.0000 +/- 0.0000 ! Units are seconds of time per year Dec_PM: 0.0000 +/- 0.0000 ! Units are seconds of arc per year Epoch: 1982.80 Annual_Parallax: 0.0220 +/- 0.0020 Flux: V = 17.09, ! Include at least V and B-V I = 13.86 Comments: from RHY sample ! This is a template for a single visit containing a single exposure ! Repeat exposure and visit blocks as needed Visits ! Section 6 Visit_Number: 01 Visit_Requirements: PCS MODE Fine ! Section 7.1 On_Hold_Comments: Visit_Comments: Exposure_Number: 10 ! Section 6.5 Target_Name: RHY067 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY067 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 02 Visit_Requirements: PCS MODE Fine ! Section 7.1 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY080 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY080 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 03 Visit_Requirements: PCS MODE Fine ! Section 7.1 On_Hold_Comments: Exposure_Number: 10 ! Section 6.5 Target_Name: RHY083 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY083 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 04 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY098 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY098 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 05 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY110 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY110 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 06 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY115 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY115 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 07 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY126 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY126 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 08 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY166 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY166 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 09 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY199 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY199 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 10 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY202 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY202 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 11 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY254 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY254 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Visit_Number: 12 Visit_Requirements: PCS MODE Fine ! Section 7.1 ON HOLD On_Hold_Comments: PI Wishes to examine data from visit 2 Exposure_Number: 10 ! Section 6.5 Target_Name: RHY297 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F1042M Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0 ! Section 7.2 SEQ 10-20 NON-INT Exposure_Number: 20 ! Section 6.5 Target_Name: RHY297 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F953N Wavelength: Optional_Parameters: CR-SPLIT=NO Number_of_Iterations: 1 Time_Per_Exposure: 1100S Special_Requirements: POS TARG 0, 0.506 ! Section 7.2 Comments: Data_Distribution ! Defaults indicated; change if desired Medium: 8MM ! 8MM or 6250BPI or 1600BPI Blocking_Factor: 10 ! 10 or 1 ! Only astronomers with very old 9- ! track tape drives should consider ! a blocking factor of 1 Ship_To: PI_Address ! STSCI or PI_Address or ! PI Address from Phase I is: ! ! MS 42 ! 60 Garden St ! Cambridge MA ! 02138-1516 USA ! ! Ship_Via: UPS ! UPS (2-day) or OVERNIGHT ! Overnight shipping done at PI expense Recipient_Email: ! Needed if Ship_To: is not PI_Address ! ! Let us know what you think of this template and software! ! Please send a list of your likes and dislikes to your Program Coordinator